Page 143 - Electromagnetics
P. 143

Then, since r = ˆ zz + ˆρρ, r = ˆ zz , and dl = dz ,wehave

                                                          ∞

                                                     ρ l      ˆ ρρ + ˆ z(z − z )

                                             E(ρ) =                      3/2  dz .
                                                    4π	  −∞ ρ + (z − z )
                                                              2

                                                                        2
                        Carrying out the integration we find that E has only a ρ-component which varies only
                        with ρ:
                                                                 ρ l
                                                       E(ρ) = ˆρ    .                          (3.64)
                                                                2π	ρ
                        The absolute potential referred to a radius ρ 0 can be found by computing the line integral
                        of E from ρ to ρ 0 :
                                                             ρ
                                                       ρ l   dρ     ρ l    ρ 0
                                              (ρ) =−             =     ln     .
                                                      2π	     ρ    2π	     ρ
                                                           ρ 0
                        We may choose any reference point ρ 0 except ρ 0 = 0 or ρ 0 =∞. This choice is equivalent
                        to the addition of an arbitrary constant, hence we can also write

                                                           ρ l    1
                                                    (ρ) =     ln     + C.                      (3.65)
                                                          2π	     ρ
                        The potential for a general two-dimensional charge distribution in unbounded space is
                        by superposition

                                                           ρ T (ρ )


                                                  (ρ) =          G(ρ|ρ ) dS ,                  (3.66)

                                                         S T
                        where the Green’s function is the potential of a unit line source located at ρ :

                                                            1       ρ 0

                                                  G(ρ|ρ ) =   ln          .                    (3.67)
                                                           2π     |ρ − ρ |

                        Here S T denotes the transverse (xy)plane, and ρ T denotes the two-dimensional charge
                                       2
                        distribution (C/m )within that plane.
                          We note that the potential field (3.66)of a two-dimensional source decreases logarith-
                        mically with distance. Only the potential produced by a source of finite extent decreases
                        inversely with distance.
                        Dirichlet and Neumann Green’s functions.     The unbounded space Green’s func-
                        tion may be inconvenient for expressing the potential in a region having internal surfaces.
                        In fact, (3.56)shows that to use this function we would be forced to specify both   and its
                        normal derivative over all surfaces. This, of course, would exceed the actual requirements
                        for uniqueness.
                          Many functions can satisfy (3.52). For instance,
                                                             A        B

                                                  G(r|r ) =       +                            (3.68)

                                                           |r − r |  |r − r i |
                        satisfies (3.52)if r i /∈ V . Evaluation of (3.55)with the Green’s function (3.68)repro-
                        duces the general formulation (3.56)since the Laplacian of the second term in (3.68)is
                        identically zero in V . In fact, we can add any function to the free-space Green’s function,
                        provided that the additional term obeys Laplace’s equation within V :
                                                   A
                                                                           2
                                        G(r|r ) =      + F(r|r ),       ∇ F(r|r ) = 0.         (3.69)

                                                |r − r |


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